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Hydrogen Deficient Stars and Related Objects
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Hydrogen Deficient Stars and Related Objects

The first helium star was discovered in 1942, the first scientific meeting on the subject, however, took place in 1985. It becomes less manifest in cool stars, where the temperature is too low to excite helium and where one has to devise indirect methods for proving hydrogen deficiency.
Undertittel
Proceeding of the 87th Colloquium of the International Astronomical Union Held at Mysore, India, 10–15 Nevember 1985
Opplag
Softcover reprint of the original 1st ed. 1986
ISBN
9789401086080
Språk
Engelsk
Vekt
310 gram
Utgivelsesdato
13.10.2011
Forlag
Springer
Antall sider
528